@Article{SantosASTSAPM:2023:NuInOr,
author = "Santos, Leonardo Barbosa Torres dos and Almeida J{\'u}nior, Allan
Kardec and Sousa-Silva, Priscilla Andressa and Terra, M. O. and
Sanchez, Diogo Merguizo and Aljbaae, Safwan and Prado, Antonio
Fernando Bertachini de Almeida and Monteiro, F.",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Universidade Estadual
Paulista (UNESP)} and {Instituto Tecnol{\'o}gico de
Aeron{\'a}utica (ITA)} and {The University of Oklahoma} and
{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Observat{\'o}rio
Nacional (ON)}",
title = "Numerical investigations of the orbital dynamics around a
synchronous binary system of asteroids",
journal = "Revista Mexicana de Astronomia Y Astrofisica",
year = "2023",
volume = "59",
number = "1",
pages = "83--97",
keywords = "Stability, celestial mechanics, minor planets.",
abstract = "In this article, equilibrium points and families of periodic
orbits in the vicinity of the collinear equilibrium points of a
binary asteroid system are investigated with respect to the
angular velocity of the secondary body, the mass ratio of the
system and the size of the secondary. We assume that the
gravitational fields of the bodies are modeled considering the
primary as a mass point and the secondary as a rotating mass
dipole. This model allows to compute families of planar and halo
periodic orbits that emanate from the equilibrium points L1 and
L2. The stability and bifurcations of these families are analyzed
and the results are compared with the results obtained with the
restricted three-body problem (RTBP). The results provide an
overview of the dynamical behavior in the vicinity of a binary
asteroid system. RESUMEN:En este artŽ\ıculo, se investigan
los puntos de equilibrio y las familias de Žorbitas periŽodicas en
la vecindad de los puntos de equilibrio colineal de un sistema
binario de asteroides con respecto a la velocidad angular del
cuerpo secundario, la relaciŽon de masa del sistema y el tamano
del secundario. Suponemos que los campos gravitatorios de los
cuerpos se modelan asumiendo el primario como punto masa y el
secundario como dipolo de masa giratorio. Este modelo permite
calcular familias de Žorbitas planas y periŽodicas de halo que
emanan de los puntos de equilibrio L1 y L2. Se analiza la
estabilidad y bifurcaciones de estas familias y se comparan los
resultados con los obtenidos con el problema de los tres cuerpos
restringido (RTBP). Los resultados brindan una descripciŽon
general del comportamiento dinŽamico en la vecindad de un sistema
binario de asteroides.",
doi = "10.22201/ia.01851101p.2023.59.01.05",
url = "http://dx.doi.org/10.22201/ia.01851101p.2023.59.01.05",
issn = "0185-1101",
label = "lattes: 2800034267415426 1 SantosJSTSAPM:2023:NUINOR",
language = "pt",
targetfile = "RMxAA..59-1_lsantos-V.pdf",
urlaccessdate = "09 maio 2024"
}